NGC 2282

0.24 UTI

0.75

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.51

C_dup

N₅₀ (P>50% members) 105

Stellar density (N₅₀/rad) 44.1 [N/pc²]

C3 classification AC

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.51 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

NGC 2282 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close

Lada & Lada (2003)
Embedded cluster within ∼2 Kpc of the Sun.

Data

🔍 Search references for NGC 2282 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	101.717	1.321	0.528	-1.085	0.329	28.859
Lada & Lada	2003	101.713	1.315	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	1.7	–	–	–	–	170	–	–
Lada & Lada	2003	1.70	–	–	–	–	170	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
VDB 85	48.6	101.74	1.35	0.55	-0.98	0.38	28.86	0.73

💡 Note: The % column shows the percentage of members that NGC 2282 shares with each listed object.

Visualization

ℹ️